Galaxy Clustering in the DEEP2 Redshift Survey

Details Galaxy Clustering in the DEEP2 Redshift Survey Galaxy Clustering in the DEEP2 Redshift Survey

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...20310604c&link_type=abstract

American Astronomical Society Meeting 203, #106.04; Bulletin of the American Astronomical Society, Vol. 35, p.1376

Astronomy and Astrophysics

Astronomy

Scientific paper

I will discuss early results from the DEEP2 Redshift Survey on galaxy clustering at z 1 as a function of color, spectral type and luminosity. We find that red, absorption-dominated, passively-evolving galaxies are more strongly clustered than blue, emission-line, actively star-forming galaxies. Intrinsically brighter galaxies also cluster more strongly than fainter galaxies at z 1. We find that the galaxy bias for the DEEP2 sample is 1.0-1.2. I will also discuss measurements of angular galaxy correlations in our DEEP2 photometric data and the dependence of galaxy clustering on redshift and color, focusing on the evolution of clustering from z 0-1.

Affiliated with

Also associated with

No associations

Rating

Galaxy Clustering in the DEEP2 Redshift Survey does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Galaxy Clustering in the DEEP2 Redshift Survey, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Galaxy Clustering in the DEEP2 Redshift Survey will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1422269